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Surface integral

Integration over a non-flat region in 3D space

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Through Mathematics, Integral and Function (mathematics)

Surface integrals have applications in physics, particularly in the classical theories of electromagnetism and fluid mechanics.

Surface integrals of scalar fields

Assume that f is a scalar, vector, or tensor field defined on a surface S. To find an explicit formula for the surface integral of f over S, we need to parameterize S by defining a system of curvilinear coordinates on S, like the latitude and longitude on a sphere. Let such a parameterization be r(s, t), where (s, t) varies in some region T in the plane. Then, the surface integral is given by

∬SfdS=∬Tf(r(s,t))‖∂r∂s×∂r∂t‖dsdt

where the expression between bars on the right-hand side is the magnitude of the cross product of the partial derivatives of r(s, t), and is known as the surface element (which would, for example, yield a smaller value near the poles of a sphere, where the lines of longitude converge more dramatically, and latitudinal coordinates are more compactly spaced). The surface integral can also be expressed in the equivalent form

∬SfdS=∬Tf(r(s,t))gdsdt

where g is the determinant of the first fundamental form of the surface mapping r(s, t).

For example, if we want to find the surface area of the graph of some scalar function, say z = f(x, y), we have

A=∬SdS=∬T‖∂r∂x×∂r∂y‖dxdy

where r = (x, y, z) = (x, y, f(x, y)). So that ∂r∂x=(1,0,fx(x,y)), and ∂r∂y=(0,1,fy(x,y)). So,

A=∬T‖(1,0,∂f∂x)×(0,1,∂f∂y)‖dxdy=∬T‖(−∂f∂x,−∂f∂y,1)‖dxdy=∬T(∂f∂x)2+(∂f∂y)2+1dxdy

which is the standard formula for the area of a surface described this way. One can recognize the vector in the second-last line above as the normal vector to the surface.

Because of the presence of the cross product, the above formulas only work for surfaces embedded in three-dimensional space.

This can be seen as integrating a Riemannian volume form on the parameterized surface, where the metric tensor is given by the first fundamental form of the surface.

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